SPICE and the art of preamplifier design
Part 1: Background
by Norman L. Koren
Updated Sept. 18, 2001
Vacuum tube audio page | Photography page
Feedback and Fidelity | Improved vacuum tube models for SPICE simulations

Table of
Part 1
Introduction | Design goals
Negative feedback | RF interference
Inverse RIAA network | Interpretation of figures
Original PAS phono preamp | Line amplifier
Modification history | References
Part 2
New phono preamp | Line amplifier choices
Line amplifiers: Purist (no tone controls)
With tone controls | Construction tips
With rotary switch tone controls
Purist II: no global feedback | Conclusions
Using PSpice
This page is adapted from an article that originally appeared in Glass Audio, Vol. 9, No. 2, p. 1 and No. 4, p. 38, 1997. Internet links have been added. Circuits with current regulator diodes for linearizing the output have been eliminated because the small reduction in low order harmonic distortion was offset by a significant increase in noise-- overall sound quality was degraded. A design with rotary switch tone controls has been added.

Portions of the material here are repeated in Feedback and Fidelity, which was intended for a more popular and less technical publication than Glass Audio.


A central mystery of high-end audio amplifier design is the poor correlation between subjective sound quality and conventional measurements (frequency response, harmonic distortion, etc.). For this reason, many of the choices involved in amplifier design-- the selection of the overall circuit topology, the use of negative feedback (NFB) and the often-overlooked tradeoff between frequency response extension and radio frequency (RF) interference-- have remained an art. Highly accurate new vacuum-tube models1 make the SPICE circuit analysis program2-4 into a powerful tool for examining inner details of tube amplifier performance. With SPICE, you can make unconventional "measurements" on your computer that would be difficult and costly with hardware instrumentation. By correlating these new measurements with careful listening, the gap between the art and science of amplifier design can be narrowed.

In this article we use SPICE to design preamplifiers of exceptional quality.  The platform for experimentation was the venerable Dynaco PAS.5  So yes, we must confess that this article contains yet another PAS modification (several, really), but the emphasis will be on insight into the design rather than on construction details. All observable flaws of the original PAS have been eliminated, and we have even been able to replace the unobtainable tone controls (in the line amplifier versions that use them) with easy-to-find linear potentiometers. The most important construction details-- the chassis and power supply modifications-- have been presented previously5 and will only be summarized here.

The simulations in this article were run on the PSpice evaluation package, which consists of Schematics for entering circuits, PSpice for simulating them, Probe for viewing the simulation results. LTspice can apparently be used for these models. Appendix A contains some tips on running Pspice. Duncan Munro has a list of SPICE vendors that could contain some hidden treasures. Current versions of PSpice may enforce the maximum number of components more rigorously than the version I've been using, 6.3.  All schematics in this article should run on current versions, but I've had circuits rejected by 7.1 that ran on 6.3.

Design goals

To create a successful product, a designer must have a set of goals and a viewpoint on how to reach them. These goals usually involve limitations in size, cost, and power consumption that must be met with minimal sonic compromise. Limitations impose a discipline on the design process that can lead to outstanding results. A "money-is-no-object" approach doesn't guarantee success.

The essential design goals are low distortion (sspecially high order), high headroom (the ability to produce a much larger output voltage than required to saturate power amplifiers), flat frequency response well beyond the audio range, non-inverting output polarity, and no frequency response irregularities at any stage of the circuit. I don't seek unlimited frequency response extension because I've found that RF interference picked up in the cables can cause serious sonic degradation. The preamplifier must be able to drive any reasonable load over any reasonable length of cable. This requires low output impedance and a feedback loop that remains stable under significant capacitive load.

I use negative feedback because it has great advantages and no drawbacks when properly implemented in a preamplifier. I design for high input impedance in each gain stage because it allows the use of small coupling capacitors, which have high self-resonant frequencies, well above the frequency range where they can affect the feedback loop. I've taken special pains to minimize the effects of RF interference introduced from the cables. I didn't use the highly linear mu-follower circuit, which operates with the full gain (mu) of the tube (too much gain in many cases and variable from tube to tube) because the compatible type of negative feedback reduces input impedance. I minimize the effect of electrolytic capacitors, which are highly nonlinear at best, in the signal path by configuring the tubes to draw for zero net ac current (or close to it) from each power supply tap.

The principal limitation imposed on the design was that it had to be constructed on a Dynaco PAS chassis using the original power transformer, whose high voltage winding is specified at a wimpy 10mA. I squeezed a little extra current out of it by using a separate filament transformer mounted on the back,5 but I was still limited to six tubes (two in new sockets mounted in chassis holes behind the line amplifier PC board). The tubes must be 12AX7s, which perform well at plate currents around 1mA, lower than other popular tubes used in preamplifiers (12AT7, 12AU7, 6DJ8). The 12AX7 is ideal for use with negative feedback (local or global) because of its high amplification factor (mu). A high-mu tube with NFB has much more precisely controlled gain than a low-mu tube without NFB.

I'm skeptical about the advantages of super-premium parts in well-designed circuits, although I use good quality parts- polypropylene capacitors, metal film resistors, etc. I believe that when it comes to designing for optimum sound quality, the magic is in the circuit.

I'm pleased to report that with the help of SPICE modeling, all the design goals have been met with no compromises. The only limitation is that it doesn't have enough gain for low output moving coil cartridges, but its performance with high output cartridges is so outstanding that many listeners may not be tempted.

Negative feedback (NFB)

Much of the material in this and the next sections is covered in greater detail in Feedback and Fidelity.
The advantages of negative feedback are well-known:  It extends frequency response, reduces distortion, allows precise control of gain, reduces output impedance and decreases a circuit's sensitivity to component variations. Nevertheless, its audible side-effects can be so bothersome that it's fallen out of favor with many audiophiles. We have identified three side-effects.

The first is that NFB causes clipping to become much more abrupt as an amplifier is driven into saturation: the greater the feedback the harsher the clipping.  This can result in the generation of really nasty sounding high order harmonics. For this reason feedback must be applied sparingly in power amplifiers.  Saturation is not an issue in the modified PAS because of its enormous headroom. It can put out up to 50VRMS into high impedance loads (over 75k). The 1.27mA dc current drawn by the output cathode follower allows it to source roughly 0.0012RLOAD V(0-Peak) = 0.00085RLOAD VRMS into low impedance loads.  Even with an extremely low load of 5k (driving two power amplifiers, each with a low 10k impedance: a worst case for biamplified speakers), the PAS can put out 4.25VRMS: well above the 1VRMS that can drive most power amplifiers into saturation.

The second side-effect of NFB is that it reduces an amplifier's stability. Poor stability is expressed as a low phase margin, the amount of additional phase shift (which could result from capacitance shunting the load) needed to drive the amplifier into oscillation. An amplifier with poor phase margin will have a high frequency peak in its frequency response and will ring in response to transient signals, especially when driving difficult, i.e., reactive loads. This ringing can cause sonic degradation.  The capacitance of long output cables (20-40pF per foot) is sufficient to cause ringing in the unmodified PAS. There are several well-known circuit techniques for stabilizing feedback loops. The original PAS uses the most common of them: 33pF capacitor CLFB in shunt with 47kilohm feedback resistor RLFB (Fig. 1). As we shall see, this "solution" is something of a Trojan Horse! We shall describe a superior technique that has no discernible ill-effects.

Radio frequency (RF) interference

The third and least-known side-effect of NFB is that the circuit technique most often employed to stabilize feedback loops, the capacitor in shunt with the feedback voltage divider resistor as described above, allows RF signals picked up by the output cable to be fed back to the amplifier input virtually without attenuation.  We have found that RF interference causes more significant sonic degradation than such better-known phenomena as harmonic distortion or frequency response irregularities.  Every circuit modification we have made to reduce an amplifier's susceptibility RF interference has made it sound smoother, sweeter, more pleasant, and more generally listenable.  This has lead us to believe that "grittiness", "graininess", "harshness", "listener fatigue", and countless other descriptive epithets that plague amplifiers with otherwise excellent specifications are largely due to RF interference.

RF interference is caused by a wide variety of sources:  radio, TV, cellular phones (with digital on the way), microwave ovens, lamp dimmers, flourescent lights, and digital appliances such as computers and CD players.  (It is particularly difficult to eliminate inside CD players, where it may be as responsible as jitter for "digititis.")  It is virtually omnipresent in urban, suburban, and all but the most remote rural areas.  It varies from time-to-time and place-to-place, and may be responsible for many of the discrepancies in published amplifier reviews.

The exact mechanism by which RF interference degrades audio quality is not well-understood.  The most likely cause is intermodulation distortion.  Paul Miller6 described a series of experiments in which he inserted strong RF signals (swept to 200MHz) modulated with random audio noise (0-20kHz) into several amplifiers, and measured the resulting audio noise spectra.  He claimed to find a strong correlation between the measured noise spectra and an amplifier's subjective sound quality.  Although RF interference is occasionally mentioned in audiophile media7, it tends to get lost among dubious tweaks.  There is a very simple test for determining if an amplifier is overly sensitive to RF interference:  Turn the volume up and listen for a pop when you turn a nearby appliance on and off.  A well-designed amplifier will remain silent.

There are five paths through which RF can enter an amplifier:  (1) direct radiation, (2) power lines, (3) internally generated by digital circuitry or rectifiers8, (4) the input cable, and (5) the output cable (potentially the most serious in feedback circuits, and certainly the most neglected).  Direct radiation (1) should have little effect on the well-enclosed PAS.  RFI power line filters (for example, Mouser part 562-851-03/3) can be quite effective with (2).  Internally-generated noise (3) is minimized by the use of fast recovery rectifiers.  We shall deal with (4) and (5) later in this article, taking full advantage of SPICE's ability to simplify measurements that would be difficult to perform in hardware, especially with signal generators and oscilloscopes that have limited frequency response.

Inverse RIAA network

A highly accurate inverse RIAA network (upper-left in the schematic below) has been used to obtain the phono preamplifier frequency response. This network has poles at 500Hz and 500kHz and zeros at 50Hz and 2122Hz. The 500kHz pole (not a part of the RIAA specification) is required because the total number of poles must be equal to or greater than the number of zeros in a realizable passive equalizer. Without it, the network output would increase by 6dB per octave forever. The output of this network differs from an ideal inverse RIAA network by -1dB at 250kHz and -3dB at 500kHz.

Although this network is realizable and well-suited for SPICE simulations, it has considerable insertion loss: -50.58dB at 1kHz and -70.5dB at very low frequencies. A somewhat more practical inverse RIAA network with less insertion loss has an upper pole at 100kHz, resulting in a -1dB error at 50kHz. It can be constructed by substituting the following values:  RIV2 = 2.2MEG (unchanged), RIV3 = 182k, CIV1 = 1450pF (560 // 560 // 330pF suggested, where // denotes components in parallel), CIV2 = 412pF (390 // 22pF suggested), and RIV4 = 5360. RIV1 includes the signal generator impedance: The values of RIV1 and RIV4 are not critical, but the values of RIV2, RIV3, CIV1, and CIV2 are quite critical and should be measured individually on a multimeter. Parallel capacitors and series or parallel resistors should be used to obtain values within about 1%.

ELAPLACE  The Laplace transform part may be used as a substitute for the inverse network. It has two advantages: (1) It's an exact implementation of the inverse RIAA network with no high frequency error. (2) It uses fewer parts-- important if you run into evaluation PSpice limits. But if you want to build a network for testing you'll have to use the RC network described above. The illustration on the right shows the use of ELAPLACE. Poles T1 and T2 and zero T3 may be entered by double clicking on the PARAM part and entering the following data.
Name  Value
VALUE1  3180e-6
VALUE2  318e-6
VALUE3  75e-6
  ELAPLACE example (Laplace transfer part) for inverse RIAA

Interpretation of figures

All figures except the photographs were created by the PSpice Schematics or Probe programs. The bias voltage indicators (e.g., 146.17 in Fig. 1) were created with the VIEWPOINT part. The circles that resemble meters are current probes created with the IPROBE part. They indicate current in amperes: 3.275E-03 is 3.274mA. The .PARAM statement required for parametric tone control runs (Figs. 3, 12) was created with the PARAM part. Tube and node designations are consistent in all figures. Table 1 describes the traces used in response curves.
VDB(LINE_IN) Phono preamplifier response.
VDB(LINE_OUT) Total amplifier response (including phono).*
VDB(LINE_OUT)-VDB(LINE_IN) Line amplifier response.*
VDB(3P)-VDB(LINE_IN) Response at line amplifier input stage plate, realtive to input.*
Table 1. Traces used in the response curves
* indicates volume control set to half (-6 dB: worst high frequency response)

Original PAS phono preamplifier and line amp
Original PAS schematic diagram

Original PAS phono preamplifier

The original PAS phono preamp (shown above) has good frequency response in the audio band (PHONO STAGE, below) except for a 2dB peak around 25Hz. It has an open-loop gain of 67.7dB, attained with the help of positive feedback resistor RPFB = 47k connected between the cathodes of the first and second gain stages (nodes 1C and 2C). Positive feedback is generally undesirable because it exacerbates the differences between tubes, i.e., open loop gain can vary by more than the tubes themselves. Without RPFB, the open loop gain drops by 4.4dB to 62.3dB. Since the preamp gain is 61dB around 25Hz, negative feedback is nearly absent at low frequencies. This means that the low frequency response is very sensitive to tube variations and can be different for different versions of the 12AX7 (suffixes A, B, WB, etc.). Mercifully, the response will become flatter- for a while- as tubes age and increased plate resistance reduces circuit gain. The poor low frequency control of the phono preamp is partly responsible for the PAS's reputation of having flabby bass. The new design completely cures these problems.
Original PAS frequency response
Original PAS frequency response

Original PAS line amplifier

The original PAS line amplifier) has many flaws not apparent from its specifications (10-40 kHz 0.5 dB; 0.05% distortion at 2V output). Chief among them is a subsonic resonance around 0.4 Hz, close to the frequency of record warps.10  This resonance is difficult to measure because most signal generators don't go low enough and because it isn't very evident at the preamplifier output (LINE_OUT). It appears in the response curve as a 40dB peak (relative to 1kHz) at the first gain stage plate (node 3P), where it can cause envelope modulation and time-varying distortion, both of which degrade imaging and overall audio quality. It may have contributed to a grindy sound I heard on LP's. It also contributes to the PAS's reputation for flabby bass.

The audio signal at the first gain stage plate (node 3P) is about 1dB below that of  the grid (node 3G)-- relatively weak in relation to RF interference from the cables introduced through the feedback loop (CLFB). This could cause sonic degradation. The signal in the first stage is attenuated because the line amplifier's closed loop gain, which is controlled by voltage divider RLFB, R3C, is less than the gain of the second stage (TU4). We correct this problem in the modified PAS by reducing the gain of the second stage with local feedback.

The output stage (TU4) is severely overloaded. Its plate resistance is around 60k, but its total load is only 20k (47k (feedback loop) // 100k (plate R) // 50k (internal + external load: 510k // 62k // 470k = 50k))  This reduces gain by about 12dB and significantly increases distortion. Negative feedback keeps the harmonic distortion figure within specification, but residual intermodulation (IM) distortion may persist. Stressing a tube in this way may degrade sound quality more than the distortion statistics indicate.

In Pspice, distortion is measured by inserting signal VIN at LINE_IN. Double-click on VIN, and set the TRAN attribute to TRAN=SIN(0 1 1K) for a 1V(0-Peak) 1kHz sine wave signal for the transient analysis.  Click on Analysis, Setup..., Transient... Set Print Step to 0.1mS (unimportant), Final Time to 2mS, No Print Delay to 0, and Step Ceiling to .01mS.  Check Enable Fourier, then set Center Frequency to 1k, Number of harmonics to 9, and Output Vars to V(LINE_OUT). Click OK. The transient box should be checked. Click Close and the analysis is ready  A distortion analysis appears at the end of the output file.  The harmonic distortion of the unmodified PAS line amplifier output is 0.128% for a 1V(0-Peak) input signal and a 5.41V(0-Peak) output signal (volume control at -6dB).

Output impedance is 2k at 10kHz, rising by 20dB per decade at lower frequencies due the impedance of CBS2 and the reduced negative feedback through CBS1. High output impedance can result in significant high frequency attenuation for long cable runs. The load (not including feedback and plate resistors) on the original PAS must be very close 50k, obtained by internal 62k and 510k load resistors in parallel with the external 470k load impedance of the ST-70 or Mark 3. The original PAS cannot drive a total load lower than 50k without severe bass degradation.

The tone control range is +17.8dB/-17.1dB at 50Hz and +12.6dB/-13.4dB at 10kHz. The original tone controls- the 750k linear bass pot and the highly nonlinear 400k treble pot- are unavailable and cannot be replaced if they go bad.  Parameter PARTX expresses the treble control nonlinearity, setting treble response to flat when the controls are centered (PAR1=0.5). With the help of SPICE (and it would be hard to imagine doing it without computer simulation) we have been able to replace these pots with widely-available linear pots and to fix all other observable problems as well.

Modification history

The modified PAS preamplifier, built in 1996.Right: The modified PAS preamplifier, (re)built in 1996.

"A New Dynaco PAS Upgrade," Glass Audio, Vol. 6, No. 4, 1994, addressed several of the PAS problems. The chassis and power supply were modified  and cathode followers were added to the phono preamplifier and line amplifier. One version of the line amplifier was designed with switchable tone controls. Another-- the purist version-- was designed without them.

The power supply modifications consisted of replacing the filament supply rectifier and filter capacitor with modern compact versions to make room for two additional tube sockets behind the line amplifier circuit board, replacing the 12X4 rectifier with silicon diodes (fast recovery recommended), increasing the B+ supply capacitance, and decreasing the resistors in the B+ supply to compensate for the additional current drawn by the cathode followers. A separate filament transformer was mounted on the back of the PAS chassis so the current drawn by the two additional tubes didn't overheat the power transformer. The present modification uses the same chassis alterations and nearly the same power supply. The new power supply schematic is shown below. (I'll fix it up with PSpice one of these days.)

Modified PAS suggested power supply
Modified PAS suggested power supply

I'd make one significant change to the power supply circuit (above). I'd get rid of RS1, the 1 ohm 2W resistor used to drop the filament supply voltage to the appropriate level (around 25V for this arrangement, where pairs of tubes are wired in series), and I'd replace it with an LM317T voltage regulator circuit between the rectifiers (FR303) and the tube filaments. I would do so for reliability-- it would make the voltage across the tube filaments independent of the current. It wouldn't have much effect on sound quality. The circuit would be similar to 12.5V supply in The Emperor's New Amplifier, with CH3 and CH4 omitted. The diagram on the right is lifted from the PDF data sheet for the National Semiconductor LM317. C1 is needed only if the device is more than 6 inches from filter capacitors. C2 can be omitted since this is not a signal circuit. The output voltage is

VOUT = 1.25(1+R2/R1) + IADJ(R2)
I leave it to the reader to calculate R2. The filaments of a 12AX7, series wired, draw 0.15 A. The six tubes in this series-parallel arrangements draw 0.45 A, well under the LM317T's 1.5 A capacity. (Other versions of the LM117/317 have lower power handling capacity.) The LM317T is inexpensive and widely available (yes, you can get it at the Shack).

The '94 mod solved several problems but left others untouched. Distortion in the overloaded line stage was greatly reduced by the addition of the cathode follower and very low impedance loads could be driven, but increased open-loop gain reduced the stability of both the phono preamplifier and line amplifier.  The phono preamplifier response was still sensitive to the individual tube. The low frequency line amplifier resonance was still present. All of these problems have been fixed in the new design.

To Part 2: New preamplifier designs


  1. Norman L. Koren, "Improved Vacuum-Tube Models for SPICE Simulations," Glass Audio, Vol. 8, No. 5, 1996, p. 18.
  2. Paul W. Tuinenga, "SPICE, A Guide to Circuit Simulation & Analysis using PSpice," Prentice-Hall, 1992 or 1995.
  3. Scott Reynolds, "Vacuum-tube models for PSPICE simulations," Glass Audio, vol. 5, no. 4, 4/93 p. 17.
  4. W. Marshall Leach, Jr., "SPICE models for vacuum-tube amplifiers," J. Audio Eng. Soc. Vol 43, No. 3, March 1995, p. 117.
  5. Norman Koren, "A new Dynaco PAS upgrade," Glass Audio, vol. 6 no. 2, 2/94, p. 10.
  6. Paul Miller, "Resonances and Repercussions," Hi Fi News & Record Review, June 1989, p. 35.
  7. John Bicht interview, "Rethinking Preconceptions," Stereophile, vol. 19, no. 6, June 1996, p. 160.
  8. Rick Miller, "Measured RFI Differences Between Rectifier Diodes...," The Audio Amateur, 1/94, p. 26..
  9. Ronald M. Bauman, "Feedforward Error Cancellation," The Audio Amateur, 2/96, p. 10.
  10. Christopher Paul, "The greening of the cascade feedback pair," Glass Audio, vol. 7, no. 5, 5/95, p. 20.
  11. Tom Mitchell, "The Audio Designer's Tube Register Volume 1," Media Concepts, Norwalk, CA.
  12. Dimitri Danyuk and George Pilko, "Error Correction in Audio Amplifiers," Journal of the Audio Engineering Society, Vol. 44, No. 9, Sept. 1996, p. 721.
  13. Jimmie D. Felps, "One extra resistor fights IC op-amp oscillations," EDN, July 3, 1997, p. 129.

About the author

Norman Koren, a native of Rochester, NY, received a BA in physics from Brown University in 1965 and an MA in physics from Wayne State University in 1969. His destiny as a high-tech nomad has taken him to Boston, Philadelphia, Silicon Valley, San Diego, and most recently to Colorado, where he worked in research and development of digital magnetic recording channels through 2001.

To Part 2: New preamplifier designs
Norman Koren Vacuum tube audio page | Photography page
Feedback and Fidelity | Improved vacuum tube models for SPICE simulations
This page
was created December 8, 2003
Images and text copyright 2001-2003 by Norman Koren. Norman Koren lives in Boulder, Colorado, where he worked in developing magnetic recording technology for high capacity data storage systems through 2001. He has been involved with photography since 1964. Designing vacuum tube audio amplifiers was his passion between about 1990 to 1998.